[135.17] High-Resolution Spectroscopy of Some Very Inactive Southern Stars

We have obtained high-resolution echelle spectra of a few
dozen solar-type stars that an earlier low resolution Ca II
H & K survey suggested have modest evels of chromospheric
activity. We present H\alpha-based chromospheric activity
measures, binarity information, and Li abundances of the
sample. As expected, our spectra: confirm the low levels of
chromospheric activity; suggest that these objects are
apparently single; indicate the stars have small projected
rotational velocities; and yield low photospheric abundances
of Li. This work was supported by NSF grant AST-0086576 to
JRK.